activity
20052019
most citedNew cooling sequences for old white dwarfs

252 citations · 2.5k across the 57 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 7 cited

On the origin of white dwarfs with carbon-dominated atmospheres: the case of H1504+65

L. G. Althaus, A. H. Córsico, S. Torres +1

We explore different evolutionary scenarios to explain the helium deficiency observed in H1504+65, the most massive known PG1159 star. We concentrate mainly on the possibility that…

astro-ph2008★ 17 cited

Revisiting the theoretical DBV (V777 Her) instability strip: the MLT theory of convection

A. H. Córsico, L. G. Althaus, M. M. Miller Bertolami +1

We reexamine the theoretical instability domain of pulsating DB white dwarfs (DBV or V777 Her variables). We performed an extensive -mode nonadiabatic pulsation analysis of DB e…

astro-ph2008★ 27 cited

Evidence of thin helium envelopes in PG1159 stars

L. G. Althaus, A. H. Córsico, M. M. Miller Bertolami +2

We present evidence that PG1159 stars could harbour He--rich envelopes substantially thinner than those predicted by current evolutionary models with current estimates of mass loss…

astro-ph2007★ 108 cited

The age and colors of massive white dwarf stars

L. G. Althaus, E. García-Berro, J. Isern +2

We present evolutionary calculations and colors for massive white dwarfs with oxygen-neon cores for masses between 1.06 and 1.28 Mo. The evolutionary stages computed cover the lumi…

astro-ph2005★ 92 cited

Mass-radius relations for massive white dwarf stars

L. G. Althaus, E. García--Berro, J. Isern +1

We present detailed theoretical mass-radius relations for massive white dwarf stars with oxygen-neon cores. This work is motivated by recent observational evidence about the existe…

astro-ph2005★ 40 cited

The formation of DA white dwarfs with thin hydrogen envelopes

L. G. Althaus, M. M. Miller Bertolami, A. H. Córsico +2

We study the formation and evolution of DA white dwarfs, the progenitors of which have experienced a late thermal pulse (LTP) shortly after the departure from the thermally pulsing…